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Low Energy Electromagnetic Physics

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Title: Low Energy Electromagnetic Physics


1
Low Energy Electromagnetic Physics
  • Maria Grazia Pia
  • INFN Genova
  • Maria.Grazia.Pia_at_cern.ch
  • on behalf of the Low Energy Electromagnetic
    Working Group

http//www.ge.infn.it/geant4/lowE/
2
Overview of physics
  • Compton scattering
  • Rayleigh scattering
  • Photoelectric effect
  • Pair production
  • Bremsstrahlung
  • Ionisation
  • Polarised Compton
  • atomic relaxation
  • fluorescence
  • Auger effect
  • following processes leaving a vacancy in an atom
  • In progress
  • More precise angular distributions (Rayleigh,
    photoelectric, Bremsstrahlung etc.)
  • Improved PIXE
  • Development plan
  • Driven by user requirements
  • Schedule compatible with available resources
  • in two flavours of models
  • based on the Livermore Library
  • à la Penelope

3
Advanced Examples
Low Energy Electromagnetic Physics
  • Stefano Agostinelli
  • Henrique Araujo
  • Pablo Cirrone
  • Giacomo Cuttone
  • Maria Catarina Espirito Santo
  • Franca Foppiano
  • Stefania Garelli
  • Patricia Goncalves
  • Alex Howard
  • Ana Keating
  • Susanne Larsson
  • Jakub Moscicki
  • Michela Piergentili
  • Alberto Ribon
  • Giovanni Santin
  • Bernardo Tome
  • Stéphane Chauvie
  • Susanna Guatelli
  • Vladimir Ivanchenko
  • Francesco Longo
  • Alfonso Mantero
  • Barbara Mascialino
  • Petteri Nieminen
  • Luciano Pandola
  • Sandra Parlati
  • Luis Peralta
  • Andreas Pfeiffer
  • Maria Grazia Pia
  • Pedro Rodrigues
  • Simona Saliceti
  • Andreia Trindade
  • Paolo Viarengo

4
Activities
  • Recent physics developments
  • Testing
  • Open issues and concerns
  • Plans

5
Processes based on the Livermore Library
  • Physics models are stable
  • Small improvements in parameterisations
  • Main effort on systematic validation
  • Photon cross sections, stopping powers,
    fluorescence done
  • Next round (already started) final state
    distributions
  • Feedback from users
  • Complementary to our own validation
  • Major project for the future design iteration
  • Needs stable physics models, sound physics and
    regression testing system
  • Performance is an issue
  • Will be addresses together with the design
    iteration, based on quantitative evaluations

6
Recent development Penelope processes
7
Processes à la Penelope
  • Physics models by F. Salvat et al., implemented
    in a FORTRAN Monte Carlo code
  • the physics models have been specifically
    developed and a great care was devoted to the low
    energy description (atomic effects, etc.)
  • the (declared) lower limit is 100 eV
  • The whole physics content of the Penelope Monte
    Carlo code has been re-engineered into Geant4
    (except for multiple scattering)
  • processes for photons June 2003 release, for
    electrons December 2003 release (Luciano
    Pandola)
  • Alternative approach w.r.t. the processes based
    on the Livermore Library

8
Gamma conversion
Mean free path in Si
e- angular distr. 5 MeV g on Si
log (mfp/cm)
Livermore-based Penelope
Livermore-based Penelope
log (Energy/MeV)
Angle (degrees)
9
Rayleigh scattering
Mean free path in Pb
Angular distr. 100 keV g on Pb
log (mfp/cm)
Low Energy Penelope
Low Energy Penelope
log (Energy/MeV)
Angle (degrees)
10
Photoelectric effect
Mean free path in Cu
Mean free path in water
log (mfp/cm)
log (mfp/cm)
Low Energy Penelope
Low Energy Penelope
log (Energy/MeV)
log (Energy/MeV)
  • The cross sections are read from the database
  • Interfaced with Livermore-based atomic relaxation

11
Compton scattering
e- angular distr. 1 MeV g on water
Mean free path in water
log (mfp/cm)
Low Energy Penelope
Low Energy Penelope
Angle (degrees)
log (Energy/MeV)
  • Analytical parametrisation for the cross section
  • The model also predicts which atomic level is
    ionised
  • ? fluorescence generation (not present in
    Livermore-Compton)

12
Bremsstrahlung (electrons)
g angular distr. 1 MeV e- on Pb
g energy distr. 1 MeV e- on Pb
Low Energy Penelope
Low Energy Penelope
Angle (degrees)
Relative g energy
  • g energy spectrum f(Z,Eel) ? database (as in
    G4LowEnergyBremsstrahlung, but 32 points instead
    of 15)
  • Also the angular distribution is data-driven
  • Recent developments by V. I. not shown here

13
Bremsstrahlung (positrons)
Mean free path in water
  • It is assumed
  • g(Z,E) ? parameterised correction function,
    independent from the g energy W

log (mfp/cm)
Electrons Positrons
log (Energy/MeV)
The g energy spectrum and the angular
distribution are the same as for electrons, only
the cross section changes
14
Validation
  • Relative comparison LowE-Livermore/Penelope only
    for curiosity
  • helpful to understand effects of different
    modeling approaches
  • and to identify software bugs!
  • Validation against reference data
  • LowE-Livermore and Penelope processes both
    subject to the same validation process
  • See EM Validation talk by Barbara on Tuesday

15
New branch of development Precise angular
distributions
16
Bremsstrahlung Angular Distributions
Three LowE generators available in GEANT4 6.0
release G4ModifiedTsai, G4Generator2BS and
G4Generator2BN G4Generator2BN allows a correct
treatment at low energies (lt 500 keV)
17
Bremsstrahlung Angular Distributions
  • Open issues and news
  • Large initialization time for G4Generator2BN (see
    Physics Manual for details)
  • use of pre-calculated data (reduces
    initialization time to zero)
  • introduced in Geant4 6.1
  • Switching mechanism between different generators
  • design iteration for final state needed
  • time scale for re-implementation and test under
    discussion

18
Photoelectric Angular Distributions
  • Current status of photoelectric angular
    distributions in GEANT4
  • G4 LowE and LowE PENELOPE processes
  • The incident photon is absorbed and one electron
    is emitted in the same direction
  • as the primary photon
  • G4 Standard (à la GEANT3)
  • The polar angle of the photoelectron is sampled
    from an approximate Sauter-Gavrila
  • cross-section (for K-shell)
  • PENELOPE
  • The polar angle is sampled from K-shell
    cross-section derived from Sauter
  • The same cross-section is used for other
    photoionisation events
  • EGSnrc Controlled by a master flag IPHTER
  • IPHTER 0 (similar to G4 LowE)
  • IPHTER 1 (Sauter distribution valid for K-shell)

Both assume that azimuthal angle distribution is
uniform (no polarisation)
19
Photoelectric Angular Distributions
in progress
  • Sauter formalism is valid for light-Z, K-shell
    photoelectrons and non-polarised photons
  • In progress use a more generalized approach
    based on Gavrila theory
  • Valid for all elements
  • For photoelectrons emitted from K and L shells
    also includes the effect of the polarisation of
    the incident photon

This enhancement is of significance importance
for the design of experiments that aim to measure
the polarisation of X-rays emitted from black
holes and neutron stars
20
New development PIXE
21
PIXE
  • Calculation of cross sections for shell
    ionisation induced by protons or ions
  • Based on a theoretical model for the calculation
    of cross sections
  • M. Gryzinski, Two-Particle Collision. I. General
    Relations for Collisions in the Laboratory
    System,   Phys. Rev. vol. 138, no. 2A, 19 April
    1965
  • M. Gryzinski, Two-Particle Collision. II. Coulomb
    Collisions in the Laboratory System of
    Coordinates, Phys. Rev. vol. 138, no. 2A, 19
    April 1965
  • Implementation in Geant4 in 2002
  • Verified to be intrinsically inadequate
  • New data-driven model
  • based on evaluated data library by Paul Sacher,
    1989 (compilation of experimental data
    complemented by calculations from EPCSSR model by
    Brandt Lapicki)
  • Incident proton energy between 5 KeV and 500 MeV
  • Elements from C to U
  • Generation of X-ray spectrum based on EADL
  • Uses the common de-excitation package

22
PIXE Cross section model
  • Fit to Paul Sacher data library results of the
    fit are used to predict the value of a cross
    section at a given proton energy
  • allow extrapolations to lower/higher energy than
    data compilation
  • First iteration, Geant4 6.2 (June 2004)
  • The best fit is with three parametric functions
    for different groups of elements
  • 6 Z 25
  • 26 Z 65
  • 66 Z 99
  • Second iteration, Geant4 7.0
  • Refined grouping of elements and parametric
    functions, to improve the model at low energies

23
Quality of the PIXE model
  • How good is the regression model adopted w.r.t.
    the data library?
  • Goodness of model verified with analysis of
    residuals and of regression deviation
  • Multiple regression index R2
  • ANOVA
  • Fishers test
  • Results (from a set of elements covering the
    periodic table)
  • 1st version (Geant4 6.2) average R2 0.998
  • 2nd version (Geant4 7.0) average R2 improved to
    0.999 at low energies
  • p-value from test on the F statistics lt 0.001 in
    all cases

Test statistics
Fisher distribution
24
PIXE status and future developments
  • First implementation for protons, K-shell
  • Geant4 6.2
  • preliminary model
  • Second iteration
  • improved model currently under test
  • Geant4 7.0
  • Third iteration protons, L-shell
  • time scale subject to availability of resources
  • Fourth iteration ions, K-shell
  • compilations of cross-sections limited to K-shell

25
Ongoing...
  • Regular maintenance and improvements in many
    areas
  • improved, precise calculation of range for
    hadrons and ions
  • extension of parameterised models for hadrons up
    to 8 Mev
  • improved treatment for some materials (i.e.
    graphite)
  • etc.
  • The physics testing project helped fixing bugs,
    identifying small problems, improving many
    details
  • Thanks to systematic and quantitative tests

26
Lower energy extensions
  • Old requirement (still from RD44)
  • Recurrent in interactions with users
  • Last User Workshop requirement to reach 10 eV
  • We are interested (of course)
  • We are aware it is difficult
  • An entire new set of phenomena to take into
    account
  • Are there any data available? How good are they?
  • Project for lower energy extensions currently
    explored together with ESA
  • More at next Geant4 Workshop

27
Current major activity Validation
See Barbaras talk on Tuesday
28
Main concern SPI
  • Software Process Improvement
  • Huge investment in SPI
  • Excellent response from most of the WG
  • Many young collaborators grown to appreciate
    rigorous SP
  • But also occasional spells of SPD
  • Coding without design
  • Maintaining private code, dropping regular
    maintenance
  • Undocumented test cases
  • Physics/algorithm documentation lies in the mind
    of individual developers
  • Difficult change management
  • etc.
  • Peer reviews
  • We would like to do more
  • Very much needed code review
  • Limitation time availability and geographical
    spread

but not worse than the rest of Geant4!
29
Summary
  • Validation
  • Major effort, with significant results
  • Highlighted some problems (solved or solutions
    planned)
  • Triggered various physics improvements
  • Sound testing system essential for planned design
    iteration
  • Recent developments
  • Penelope re-engineering
  • Precise angular distributions (Bremsstrahlung,
    photoelectric)
  • PIXE
  • Outlook
  • Lower E requirements to be addressed
  • Validation of existing models
  • Design and code reviews
  • SPI (continuous education to a rigorous software
    process)
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